Celestial hemisphere:  Northern  ·  Constellation: Hercules (Her)  ·  Contains:  IC 1170  ·  IC 1172  ·  IC 1178  ·  IC 1179  ·  IC 1181  ·  IC 1182  ·  IC 1183  ·  IC 1184  ·  IC 1185  ·  NGC 6039  ·  NGC 6040  ·  NGC 6041  ·  NGC 6042  ·  NGC 6043  ·  NGC 6044  ·  NGC 6045  ·  NGC 6047  ·  NGC 6050  ·  NGC 6054
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Abell 2151 Hercules Galaxy Cluster, Mau_Bard
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Abell 2151 Hercules Galaxy Cluster

Revision title: Closeup

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Abell 2151 Hercules Galaxy Cluster, Mau_Bard
Powered byPixInsight

Abell 2151 Hercules Galaxy Cluster

Revision title: Closeup

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Description

The Hercules Cluster (Abell 2151) is an impressive cluster of about 200 galaxies, distant 500 million light-years in the constellation Hercules.
It is rich in spiral galaxies and shows many interacting groups, i.e. Arp 272 (NGC 6050, IC 1179, and a third one) and Arp 71 ("integral" NGC 6045 and companion on its left tip, just visible here) and Arp 122 (NGC6040 spiral left and companion).
The brightest member is the giant elliptical galaxy NGC 6041.
The cluster is part of the larger Hercules Supercluster, which is itself part of the much larger Great Wall super-structure.
It was described by Harlow Shapley in 1933 for the first time.

The Hercules Cluster is not as rich in galaxies, nor as centrally concentrated, as the Coma cluster. Clusters of this kind may be rich in spiral and irregular galaxies, and in Abell 2151 we see many interacting galaxy pairs and small groupings of galaxies. In both the dynamics of the cluster and its galaxy population, it may be possible to view Hercules as less evolved than Coma. Recent observations show that many Coma-like clusters seen at higher redshifts (and thus as they were several billion years ago) have galaxy populations much like we see today in the Hercules cluster, with numerous spiral and interacting galaxies. Some combination of interactions, mergers, and effects of intracluster gas may be driving this change with time.

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